Fig. 11
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As Fig. 10, but for models with two dust components with density-dependent abundances. Results are shown for the cloud model C with
and density thresholds n0= 103−3.2 × 104 cm−3, with symbols for higher n0 values shifted to slightly higher y-axis positions. In frame d, τ(J) is calculated using the actual dust models and the spatially varying extinction curves. The vertical lines in frames d-e indicate the corresponding single-dust results from Fig. 10 for the first (cyan lines) and the second (magenta lines) of the dust components.
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